Results 31 to 40 of about 109,917 (327)
Martian Bow Shock and Magnetic Pile-Up Barrier Formation Due to the Exosphere Ion Mass-Loading [PDF]
Journal of Astronomy and Space Sciences, 2011 Bow shock, formed by the interaction between the solar wind and a planet, is generated in different patterns depending on the conditions of the planet.
Eojin Kim +6 more
doaj +1 more source
The Political Culture; Politicial Socialization and Acculturation
Journal of Legal Studies, 2015 In this article, the author, after having comparatively analyzed senses and significations of the concept of politic culture, as stated by several renowned authors in the world of science, proceeds to a differentiation of general political culture from ...
Iovan Martian
doaj +1 more source
Journal of Management and Business Review, 2018 Abstrak - Penilaian tingkat kinerja perusahaan pembiayaan merupakan kepentingan bagi semua pihak yang terkait (stake holder), baik pemegang saham dan pengelola perusahaan pembiayaan, pihak pengguna jasa perusahaan pembiayaan baik supplier, kreditur ...
Catur Martian Fajar
doaj +1 more source
Astrobiology, 2017 The Mars Organic Molecule Analyzer (MOMA) instrument onboard the ESA/Roscosmos ExoMars rover (to launch in July, 2020) will analyze volatile and refractory organic compounds in martian surface and subsurface sediments.
F. Goesmann +24 more
semanticscholar +1 more source
The Environmental Education Dimensions for Sustainable Development
Journal of Legal Studies, 2015 Based both on a historical approach regarding the evolution of the environmental education between 1960 and present days, and on empirical research as well, the author proves that the efficiency of the environmental education could be much higher if ...
Iovan Martian
doaj +1 more source
Interplanetary Magnetic Field Effect on the Location of the Martian Bow Shock: MAVEN Observations
The Astrophysical Journal, 2023 The Martian bow shock (BS) is generated with the mass-loading and magnetic pileup processes when the solar wind interacts with the Martian ionosphere. In this vein, the interplanetary magnetic field (IMF) frozen in the solar wind can affect the location ...
H. Y. Sui +4 more
doaj +1 more source
Morphologic Diversity of Martian Ripples: Implications for Large‐Ripple Formation
Geophysical Research Letters, 2018 Large ripples with meter‐scale wavelengths are ubiquitous across Mars. Curiosity's traverse of the Bagnold Dune Field revealed a morphologic diversity of large Martian ripples that helps constrain their formative mechanism.
M. Lapôtre +6 more
semanticscholar +1 more source
, 2017 We analyze the complete set of in-situ meteorological data obtained from the Viking landers in the 1970s to today’s Curiosity rover to review our understanding of the modern near-surface climate of Mars, with focus on the dust, CO2 and H2O cycles and ...
G. Martinez +16 more
semanticscholar +1 more source
Earth, Planets and Space, 2021 The mass spectrum analyzer (MSA) will perform in situ observations of ions and magnetic fields around Phobos as part of the Martian Moons eXploration (MMX) mission to investigate the origin of the Martian moons and physical processes in the Martian ...
Shoichiro Yokota +16 more
doaj +1 more source
Variations of the martian CO2 abundance with Martian season [PDF]
Symposium - International Astronomical Union, 1971 All previous published equivalent widths of the Martian CO2 bands including the 1967 apparition coverage at McDonald Observatory are reduced to CO2 abundances using the same curve of growth parameters. The corresponding CO2 partial pressures (assuming a pure CO2 atmosphere), along with the regression curves of the north polar cap, are presented as ...
openaire +2 more sources